Y2K Linux bug ??

1999-11-08 Thread Armel Le Bail

Hi !

The latest mails archived at :

http://www.mail-archive.com/rietveld_l@ill.fr/

are dated by January 1999... Is this already an effect
of Y2K ?

Armel Le Bail
http://www.cristal.org/



Re: Y2K Linux bug ??

1999-11-08 Thread Alan Hewat

At 11:15 08/11/1999 +0100, [EMAIL PROTECTED] wrote:
>The latest mails archived at :
>http://www.mail-archive.com/rietveld_l@ill.fr/
>are dated by January 1999... Is this already an effect
>of Y2K ?

Hmm. As you see from the header, the mails that I receive from our Rietveld
server are correctly dated (The server is a Unix machine, not Linux).  

Please check your archive set-up Armel.  It might be something to do with
the world being upside down because of the result of the rugby world cup
final :-)

Alan.

Alan Hewat, ILL Grenoble, FRANCE <[EMAIL PROTECTED]> tel (33) 4.76.20.72.13 
ftp://ftp.ill.fr/pub/dif  fax (33) 4.76.20.76.48  http://www.ill.fr/dif/



Re: [sdpd] Re: PowBase

1999-11-08 Thread Armel Le Bail

At 22:14 07/11/99 -0200, Helio Salim de Amorim wrote:

>I think that PowBase is yet a remarkable step and your public domain
>character a very important aspect.  I think also,  that is not necessary a
>hard standardization but a few directions like,
>- the data must be an ASCII file.
>- unpublished data may be accepted (these are the cases,  for example, of
>good measurements of standards or rare materials) and in this case the
>authors must include in the data file a heading (or footnote) with a
>description of relevant experimental conditions and comments about the
>sample ( that typically presented in a regular paper).
>By our part PowBase have total approve and a sincere personal thanks for the
>initiative.

Thanks a lot, it was your suggestion !

Powbase has already reached some cruising speed with 79 patterns
added in 5 days. Theoretically, 190 days would suffice for being
the equivalent of the 3000 patterns in PDF-3. Of course, 
maintaining that speed depends on you.

http://sdpd.univ-lemans.fr/powbase/

The current entry format replies to almost all recent suggestions,
and it is really the most simple I can imagine (free format).
It is not CIF nor CIF star, but those formats will be accepted too.

Best,

Armel Le Bail
http://www.cristal.org/



Re: CIF format

1999-11-08 Thread Armel Le Bail

Kurt  wrote:

>Can I dump the extracted structure factors from GSAS
>into ESPOIR, for example?  It would be nice if this was really happening...

I am not a GSAS user, but as the ESPOIR programmer, I would say
that nothing is more easy than to dump structure factors into it.

The format is free, ascii, corresponding to one line per h,k,l, "|Fobs|",
so that the following possibilities can be accepted :
200
   1 0 1  251.2
   2 2 0 348.3
...

or 
200
  1   0   1   251.20   0.52
  2   2   0   348.30   0.65
...

or more stuff unused after the "|Fobs|".

If no GSAS output fits into that format, it is surprising.

Best,

Armel Le Bail
http://sdpd.univ-lemans.fr/course/



gsas in dos & UNIX

1999-11-08 Thread Roger Mason

hello,

Does anyone know if it is possible to use the same *.EXP file on dos &
UNIX (Linux) machines?

If so, what changes must be made to the file?

Thanks in advance,

Roger Mason



Re: [Re: [sdpd] Re: PowBase]

1999-11-08 Thread Andrew Wills

Dear All,

I think that standardisation is an important topic at the moment- the dawn of
a database of diffraction patterns. If you take a look through the different
formats that GSAS and FULLPROF can accept (I name those only for convenience)
it is a bit of a jungle- I include of course both 2-axis and TOF data. This
situation has been given to us by history and the way that the Rietveld codes
were created and evolved, but it is an unnecessary complication that is easy
to get rid of. 

The powder CIF is doubtless the most sensible format for stocking data as it
details all the appropriate experimental conditions (sample holders, cryostat,
oven, etc) and whilst these and other pieces of information can be very
important, they may easily be forgotten when someone submits a data file. What
we need also is a standard set of routines (or programs) that we can all use
to convert data and experimental details to the powder cif format, and from
that to those we wish to use in the refinement. If all software authors have
to do this job the movement to this format will be very slow, and I personally
find it a pain to reinvent the wheel constantly.

Armel, how would you feel about accepting magnetic data? -are you accepting
all waifs and strays (sdf's in French)? :-) Or perhaps Alan, you would prefer
to house them at the ILL.

Sincerely,

-Andrew


>I think also,  that is not necessary a
>hard standardization but a few directions like,
>- the data must be an ASCII file.
>- unpublished data may be accepted (these are the cases,  for example, of
>good measurements of standards or rare materials) and in this case the
>authors must include in the data file a heading (or footnote) with a
>description of relevant experimental conditions and comments about the
>sample ( that typically presented in a regular paper).


---
Andrew S. Wills (Dr.)
SPSMS/DRFMC/MDN
Centre D'Etudes Nucléaires de Grenoble
17 Avenue des Martyrs
Cedex 9
Grenoble, 38054
France

email:   [EMAIL PROTECTED]



Get your own FREE, personal Netscape WebMail account today at 
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Re: [gsas in dos & UNIX]

1999-11-08 Thread Andrew Wills

Hi Roger,

I don't think that there will be problems with the EXP file, but there could
be with the data file as the end of line statements may not be there  in the
UNIX version and all the data may be on one line. If this is the case you will
simply need to convert it to an 80 column per line format for it to work in
DOS. If you do have problems, the first thing to check is that all the files
(instrument parameter, data and exp) have 80 characters per line (this is a
classic starting problem for new GSAS users). You can do this easily by
opening it in Word (or non-Bill Gates editor) and using the 'view nonprint
characters' button (the one that looks like '1P' ). There is a program in the
first menu of GSAS (I forget the name) that pads ascii files with the extra
spaces required.

I hope that this is useful,

-Andrew



Does anyone know if it is possible to use the same *.EXP file on dos &
UNIX (Linux) machines?

If so, what changes must be made to the file?

Thanks in advance,

Roger Mason



Get your own FREE, personal Netscape WebMail account today at 
http://webmail.netscape.com.



Data Format

1999-11-08 Thread P . G . Radaelli

dear all,

since standard data formats were mentioned, I would just like to draw your
attention to the NeXus project, which has the (ambitious) purpose of
developing a unified data format for x-rays and neutrons.

http://www.neutron.anl.gov/NEXUS/
http://lns00.psi.ch/NeXus/

The NeXus format is based on HDF, which is an industrial standard.  I'm not
directly involved, but I know that they specifically looked at CIF as an
alternative.  They found that, in it's native format, CIF it is not suitable
to handle large amounts of raw data.  There is, however, something called
imgCIF, which might address the problem.  I quote from the NeXus web site:

"In a round table discussion at the [NOBUGS] workshop [ILL, JAN96], we
discussed the merits of the NeXus proposal compared to a proposal to extend
CIF by including binary images (imgCIF). Those involved in the NeXus
proposal did not think that imgCIF would have sufficient flexibility to
describe complex neutron instrumentation. Those involved in the imgCIF
proposal preferred the CIF use of ASCII header information and were
concerned about HDF's ability to handle the high data rates at synchrotron
sources. We have decided not to try and merge the two proposals at this
stage, particularly since, in our view, they are serving different
purposes."

If you wonder why powder diffractionists should be concerned with large data
files, please note that the new ISIS high-flux powder diffractometer GEM, of
which I am responsible, produces about 64 Mbytes of integers (14 Mbytes when
compressed) for every data set (this will increase to ~150 Mbytes when the
instrument is complete), and we can get good-quality data in as little as 10
seconds.  This is the brave new world, gentlemen

Paolo



Re: a few words about pdCIF

1999-11-08 Thread Brian H. Toby

Lubomir Smrcok wrote:
> It would be nice if you make public the subroutines you have
> mentioned in your mail. 

Sorry, no intent to be obscure, just brief. See
http://www.iucr.org/iucr-top/cif/index.html (in the Americas,
http://www.us.iucr.org/iucr-top/cif/index.html) and look for CIFtbx2
(and CIFtbx) under software. Ignore anything about DDL2 or greater
unless you are into macromolecular work.

Brian



Re: gsas in dos & UNIX

1999-11-08 Thread Bob Von Dreele

Roger (& others),
The transfer of GSAS files from unix (linux) to PC is straightforward, but
one does have to do certain things to get it right. The problem is that
these files (exp, data & iparm) are all in fixed record length (80
character) direct access format. On unix machines this has the appearance
of one very long record with no intervening "end of record" marks while on
a PC each 80 character record is terminated by two additional bytes
(CR/LF). The safest way to tranfer these files from unix is to first use
the convdtos utility in GSAS to convert them to standard sequential file
format. Then tranfer the files (e-mail attachments or ftp) to the PC. Then
use the cnvfile utility in PC-GSAS to convert them back to 80 character
records. Do not transfer the direct access format files directly from unix
to PC as they are unreadable. 
To transfer these files from PC to unix one only need to transfer the files
(e-mail of ftp) and then use the GSAS utility convstod to make them direct
access.
I hope that helps,
Bob Von Dreele
At 09:28 AM 11/8/99 -03-30, you wrote:
>hello,
>
>Does anyone know if it is possible to use the same *.EXP file on dos &
>UNIX (Linux) machines?
>
>If so, what changes must be made to the file?
>
>Thanks in advance,
>
>Roger Mason



Re: gsas in dos & UNIX

1999-11-08 Thread Brian H. Toby

Roger Mason wrote:
> Does anyone know if it is possible to use the same *.EXP file on dos &
> UNIX (Linux) machines?
> 
> If so, what changes must be made to the file?

The file contents are exactly the same for the .EXP as well as the data
and instrument parameter files, but in DOS the records must be exactly
82 characters per line, including the CR-LF terminator. In UNIX the
files should be exactly 80 characters per line with no terminators. 

To xfer files from UNIX to DOS you need to add a terminator or else when
the files get into DOS, you have one huge record that is very hard to
work with. This can be done in UNIX with the GSAS CONVDTOS program.
(DTOS = Direct-access to Sequential). One the files are in DOS, you then
format them using the CONVERT program in GSAS that adds the CR-LF
terminator.

To go from DOS format to UNIX, run CONVSTOD.

The version of CONVSTOD/CONVDTOS that is in the current release of GSAS
is full of "features." For example, it will ruin files that are
converted twice. (My fault not Bob.) A newer version can be found at
ftp://ftp.ncnr.nist.gov/pub/cryst/gsas/cconvstod.c with compiled
versions at
ftp://ftp.ncnr.nist.gov/pub/cryst/gsas/exe_XXX/convutil.tar.gz (XXX=SGI
and linux). [Link the executable to .../gsas/exe/convstod and
.../gsas/exe/convdtos and run from the menus or from the command line as 

.../gsas/exe/convstod < input > output

The sequential files produced by this version of convdtos are in the DOS
format. It does not screw up the file, if you convert a file that is
already in the correct format.

Brian


Brian H. Toby, Ph.D.Leader, Crystallography Team
[EMAIL PROTECTED]  NIST Center for Neutron Research, Stop 8562
voice: 301-975-4297 National Institute of Standards & Technology
FAX: 301-921-9847Gaithersburg, MD 20899-8562




Re: Thin samples in Bragg-Brentano geometry

1999-11-08 Thread Bob Von Dreele

Kurt (& others),
The real problem with small samples in Bragg- Brentano geometry is assuring
that the sample covers uniformly the entire "foot print" of the incident
x-ray beam at all scattering angles used in the scan, i.e. there are no
"bare spots". If this is not achieved then the observed diffraction
intensities will bear little relation to what should be observed
(particularly at low angles). The sample thickness for typical samples
(metal oxides, say) is infinite at 20 or so microns so the problem isn't
the thickness but is ensuring the coverage.
Bob Von Dreele
At 05:44 PM 11/7/99 -0700, you wrote:
>Rietvelders,
>
>For a lot of small powder samples (say 10 milligrams) in Bragg-Brentano
>geometry, the sample has to be spread very thin over the diffracting
>surface of a slide in the diffractometer.  I notice that a lot of the
>textbook formulas are for "infinitely thick" samples.  Is there a special
>way to deal with the thin samples?  It seems like the absorption part of
>the formula for peak intensities (for example, for phase fractions in
>multiphase mixtures) will be changed.
>
>   - Kurt Leinenweber
>
>*
>Kurt Leinenweber
>Dept. of Chemistry
>Arizona State University
>Tempe, AZ  85287-1604
>
>Phone (480)-965-8853
>Fax   (480)-965-0474
>
>



Re: [Re: [sdpd] Re: PowBase]

1999-11-08 Thread Armel Le Bail

Andrew S. Wills wrote :

>Armel, how would you feel about accepting magnetic data? -are you accepting
>all waifs and strays (sdf's in French)? :-) Or perhaps Alan, you would prefer
>to house them at the ILL.

I think that sounding opinions about doing or not a database, and
asking to researchers if they are ready to share their data would
have surprising results (large percentage of "no", very probably).

So, the question is, will the base increase ? The ICDD base receives
data from ICDD members, grants in aid, essentially (?), and the
failure of this method to provide a complete database is evident
with the recent add of calculated patterns from ICSD and in a
near future from CSD.

The size of PowBase for 80 patterns is 800Ko, thanks to compression
by Winzip. A base of 3000 patterns would be 30Mo, and this is
not a problem, even on a simple PC with full Internet connection. The
same PC stores already a base of more than 1 most cited chemists
(ISI data). But clearly, ToF large data should be left at ISIS or elsewhere.
And a base of magnetic data would be self consistent at ILL. How to
manage a very simple database is explained at the PowBase Web site. 
But who wants to manage a free database apart me ?-)). Or who 
has permission to do it ? Is that possible at NIST ? Ask yourself why
such databases are so few. The Studsvisk database of amorphous
diffraction patterns (powder-like) is still underdeveloped (because
nobody sends data ?).

Now let us discuss about standard formats. Why CIF has to be
so complex ? The aim is to produce a completely self consistent
block of data which would allow to do not need the corresponding
publication at all. In fact, IUCr can almost produce automatically
a standard publication from a CIF file. And the atomic coordinates are
supposed to be included, of course. But if one considers that the
publication will be available separately, then the format has certainly
not to be so complete, and only the point by point intensities are
really needed (for a constant wavelength powder pattern). May be
you heard about PubMedCentral or E-Biomed, a free access project
for  electronic publications at NIH. It is a pity that the project was not
more general, because a big PubCentral would solve that problem : no
need for a so complete and complex CIF when publications are available
online (and for free...).

I would have one question about PDF-3. Up to now, ICDD never
produced atomic coordinates. And I guess that the World has been
commercially divided in databases with or without atomic
coordinates. So the question is, will the CIF star include atomic
coordinates inside PDF-3 ? If not, either the publication or another
database (ICSD, CSD) will be needed, eventually, if more than
an identification of a compound is the target.

Best,

Armel Le Bail
http://sdpd.univ-lemans.fr/powbase/

Armel Le Bail - Universite du Maine, Laboratoire des Fluorures,
CNRS ESA 6010, Av. O. Messiaen, 72085 Le Mans Cedex 9, France
http://www.cristal.org/



Re: Data Format

1999-11-08 Thread Brian H. Toby

[EMAIL PROTECTED] wrote:
> I would just like to draw your
> attention to the NeXus project, which has the (ambitious) purpose of
> developing a unified data format for x-rays and neutrons.
> http://www.neutron.anl.gov/NEXUS/
> http://lns00.psi.ch/NeXus/

The NeXus format is an excellent way to deal in binary with the large
amounts of data generated by many energy-dispersive and PSD instruments.
CIF stinks for this and my impressions are that imgCIF is a Band-Aid
that is far less versatile than NeXus. NeXus is also designed for other
types of scattering experiments than diffraction.

The unanswered question that faces the powder-diffraction
crystallographic community is, if crystallographers standardize on CIF
for communication of structural results (pretty much a fact already) and
major neutron and x-ray sources standardize on NeXus (pretty likely),
how does the gap get bridged?

Brian


Brian H. Toby, Ph.D.Leader, Crystallography Team
[EMAIL PROTECTED]  NIST Center for Neutron Research, Stop 8562
voice: 301-975-4297 National Institute of Standards & Technology
FAX: 301-921-9847Gaithersburg, MD 20899-8562




RIET: Re: [sdpd] Re: Use of CIF as advocated by Lachlan

1999-11-08 Thread L. Cranswick


(keeping the entire text of Robin's Email as it was not
Cc'd to the Rietveld list).

Robin Shirley ([EMAIL PROTECTED]) writes: 
> Lachlan Cranswick writes [Fri, 5 Nov 1999 17:59:40 + (GMT)]:
> 
> > While the database system Armel has done looks good,,
> > this still leaves the problem of a common file
> > format.  If CIF was used, many of the problems/requests
> > described by Andrew would become non-issues.
> 
> I'm reluctant to take issue with Lachlan, who does such a good job at 
> the CCP14 website, and indeed publishes CRYSFIRE from there.
> 
> However, I have to say that I'd feel happier about supporting CIF as a common
> file format if (a) it were considerably simpler to read and (b) the CIF
> committee were more responsive to practical powder-related issues.
> 
> Firstly let me say that, in a spirit of general co-operation, several years
> ago I extended CRYS/CRYSFIRE to support a basic form of CIF as a file-save
> option (i.e. for output).
> 
> However I can't support it as an input format due to its excessive
> complexity.  I simply don't have the address space available in CRYS, and
> most of what's included in CIF would be irrelevant for this purpose.
> 
> Also, my attitude is partly coloured by the fact that, both at Beijing in 
> 1993 and at Seattle in 1996, I submitted a formal proposal concerning a small 
> set of Powder-CIF extensions which would cover issues connected with indexing
> (copies emailed on request), as at present these are not touched on.
> 
> On each occasion I took the precaution of first running them past Brian Toby 
> to confirm that their syntax was well formed.  And both times absolutely 
> nothing happened.  I didn't even receive the courtesy of an acknowledgement.
> 
> Brian told me at Seattle that the committee seemed to have lost the 1993
> proposals.  After resubmitting them, I again got no reply, so I didn't bother
> trying again at Edinburgh.
> 
> In the light of this, I'm afraid that as a software author I don't feel
> encouraged to put myself out to support CIF as a common file format, when
> the CIF committee rather gives the impression of living in an ivory tower 
> remote from actual users.
> 
> Robin Shirley
> School of Human Sciences
> University of Surrey
> UK
> 

For a sizable database, I don't see an alternative to CIF
for being able to transfer Crystallographic structure
and data information in a civilised manner (?)
(compared to having a dozen or so different formats where
things could become a mess quite quickly).   If not CIF,
then what?

(Does NEXUS just handle data - or can it include structure
information?)

-

On the single crystal side, Louis Farrugia's CIF conversion
software is very solid; showing good CIF conversion can be done,
both in converting "structure" and "reflection" data into
WinGX's shelx format.
http://www.chem.gla.ac.uk/~louis/software/
http://www.ccp14.ac.uk/ccp/web-mirrors/farrugia/~louis/software/
http://ccp14.sims.nrc.ca/ccp/web-mirrors/farrugia/~louis/software/

How much programming effort (hours, days?) would it considered
standard to be able to program in a CIF to X converter for
say GSAS or Fullprof, or X?  Is any source code available that
could be used as a template for powder authors?

Is there any instance of a powder program being able to
import a CIF into the program's native powder format?

Lachlan.

PS: With respect to Robin's comments on trying to get additions
to PowderCIF for Powder Indexing,;what is the present mechanism
for getting things implemented into the Powder CIF area?


-- 
Lachlan M. D. Cranswick

Collaborative Computational Project No 14 (CCP14)
for Single Crystal and Powder Diffraction
Daresbury Laboratory, Warrington, WA4 4AD U.K
Tel: +44-1925-603703  Fax: +44-1925-603124
E-mail: [EMAIL PROTECTED]  Ext: 3703  Room C14
   http://www.ccp14.ac.uk



Re: Data Format - GEM and 64 Mbyte datasets

1999-11-08 Thread Lachlan Cranswick


[EMAIL PROTECTED] Wrote:
At 13:47 08/11/99 -, you wrote:
>dear all,
>If you wonder why powder diffractionists should be concerned with large data
>files, please note that the new ISIS high-flux powder diffractometer GEM, of
>which I am responsible, produces about 64 Mbytes of integers (14 Mbytes when
>compressed) for every data set (this will increase to ~150 Mbytes when the
>instrument is complete), and we can get good-quality data in as little as 10
>seconds.  This is the brave new world, gentlemen
>
>Paolo

Is there GEM related information on available software (or portability
tools) that are being developed in parallel with the hardware so that GEM 
can produce "usable" and "analyzable" data?  Users might consider it a 
backward step to have diffraction hardware that produces 64 Mbyte datasets - 
where present available analysis software is more optimised for files 
measured in Kbytes?

Lachlan.

Lachlan M. D. Cranswick

Collaborative Computational Project No 14 (CCP14)
for Single Crystal and Powder Diffraction
Daresbury Laboratory, Warrington, WA4 4AD U.K
Tel: +44-1925-603703  Fax: +44-1925-603124
E-mail: [EMAIL PROTECTED]  Ext: 3703  Room C14
   http://www.ccp14.ac.uk



RE: Data Format - GEM and 64 Mbyte datasets

1999-11-08 Thread P . G . Radaelli

Lachlan:

>Is there GEM related information on available software (or portability
>tools) that are being developed in parallel with the hardware so that GEM 
>can produce "usable" and "analyzable" data?

Yes, we have a major software effort to handle these data and reduce them
down to manageable sizes.  Files will still be quite a lot bigger than  CW
files, because we have the wavelength and angle information which come out
separately, but I am aiming at something like 500Kbites uncompressed (7
patternsx3000 time channelsx 32 bytes of data/errors).  The problem is that
the reduction algorithms are not set in stone.  The user must be able to
interact with the software and select the optimal way to combine detectors
into groups.  Our answer to this challenge, for the moment, is and IDL based
platform called ARIEL, which also has some fortran bits for added speed.  It
was designed to be instrument-independent, so it can handle all the ISIS
diffractometers, and, hopefully, other institutions as well.  We have
acquired the right to distribute IDL executables free of charge even for the
users who don't have IDL.

Still, this means serious multi-histogram Rietveld (7 patterns or sometimes
more).  To make things simpler for the users, I will try to produce data
normalised on an absolute cross-section scale, so that the histogram scales
can be all set to the same value.  I'm sure this is possible, because it's
done routinely for liquid-amorphous scattering.  Also, I would aim at having
all the patterns on the same Q scale, so that the instrument parameters do
not need to be refined.  ARIEL is designed to do all these things, but we
are not quite there yet.

The fast data output poses even more challenges.  Ultimately, Rietveld code
will need to be updated to cope with all this.

Paolo



Re: RIET: Re: [sdpd] Re: Use of CIF as advocated by Lachlan

1999-11-08 Thread Brian H. Toby

Robin Shirley ([EMAIL PROTECTED]) writes:
> However, I have to say that I'd feel happier about supporting CIF as a common
> file format if (a) it were considerably simpler to read and (b) the CIF
> committee were more responsive to practical powder-related issues.

I do owe Robin an apology for my inaction. I have still not completed
all the tasks I have promised with respect to pdCIF v1.0 and so I have
not started work on v1.1, which will incorporate some of the additions
suggested by Robin and others. CIF is something that I work on at home,
not as part of my employment and time for it is scarce. A volunteer to
take over for me would be very welcome.

L. Cranswick wrote:
> PS: With respect to Robin's comments on trying to get additions
> to PowderCIF for Powder Indexing,;what is the present mechanism
> for getting things implemented into the Powder CIF area?

As of right now, the procedure is to read through the pdCIF dictionary
to determine what it is you want to store that is not present and then
define the term to be added. You then write to me with a case for why
the terms are necessary and then let your e-mail age in CIF inbox for a
while. A IUCr committee (pdDMG) will eventually evalute these
suggestions. I hope to be ready to start this soon.

I would like to note that while there is a lot of information that can
be stored in a powder CIF, software that reads CIFs needs only to deal
with the relevant fields for the task at hand and can ignore the rest.
While CIF has provisions for including structural information, peak and
reflection tables,... life does not need to be so complex. For storage
of raw lab data, one can write a very simple CIF file that looks like
this:

data_myCIF

_pd_meas_2theta_range_min  5.0
_pd_meas_2theta_range_max  65.0
_pd_meas_2theta_range_step 0.02

loop_  _pd_meas_counts_total
10 16 23 18 ...

That's it! Not so complex.

Of course it would be a good idea to use the appropriate CIF terms to
describe if the data are x-ray or neutron, specify wavelengths used, if
a theta-compensating slit was used,... As many people keep
rediscovering, ambiguous data can be very hard to use.

> (Does NEXUS just handle data - or can it include structure
> information?)

There is no reason that NeXus could not include any kind of information,
but no provisions exist as far as I know. It is really being implemented
as a raw data format.

Brian
 

Brian H. Toby, Ph.D.Leader, Crystallography Team
[EMAIL PROTECTED]  NIST Center for Neutron Research, Stop 8562
voice: 301-975-4297 National Institute of Standards & Technology
FAX: 301-921-9847Gaithersburg, MD 20899-8562




Advice on a new diffractometer

1999-11-08 Thread Kurt Leinenweber

Hi everyone,

There is a diffractometer here for rapid data collection (Siemens D5000,
7.5 degree position-sensitive detector, no monochromator and can't be
retrofitted for one).

My question is, what would be a good choice for a second diffractometer in
this situation (ie what brand, what kind of monochromators and detectors,
etc)?  I am hoping to be able to collect data that can be used to find unit
cells and do refinements, perform Monte Carlo solutions for complex phases,
etc.  The PSD system is not very good for this (it even has K-beta bumps
that come through the nickel filter!) Thanks!

- Kurt Leinenweber

*
Kurt Leinenweber
Dept. of Chemistry
Arizona State University
Tempe, AZ  85287-1604

Phone (480)-965-8853
Fax   (480)-965-0474





rietveld_l@ill.fr

1999-11-08 Thread Le Bail Armel

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From: Armel Le Bail <[EMAIL PROTECTED]>
Subject: Re: Advice on a new diffractometer
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>My question is, what would be a good choice for a second diffractometer in
>this situation (ie what brand, what kind of monochromators and detectors,
>etc)?  

Try "NIST" as keyword in PowBase, you will obtain 2 patterns which
are the best you can do in a laboratory, and a link to a discussion
on that question and to more demonstration patterns.

Armel Le Bail
http://sdpd.univ-lemans.fr/powbase/